Difference between revisions of "Documentation/4.8/Modules/AstroSmoothing"
(Nightly -> 4.8) |
m (Text replacement - "\[http:\/\/www\.slicer\.org\/slicerWiki\/index\.php\/([^ ]+) ([^]]+)]" to "$2") |
||
Line 26: | Line 26: | ||
* Thijs van der Hulst, <email>J.M.van.der.Hulst@astro.rug.nl</email> | * Thijs van der Hulst, <email>J.M.van.der.Hulst@astro.rug.nl</email> | ||
* Jos Roerdink <email>j.b.t.m.roerdink@rug.nl</email> | * Jos Roerdink <email>j.b.t.m.roerdink@rug.nl</email> | ||
− | [ | + | [[Documentation/Nightly/Extensions/SlicerAstro|Back to SlicerAstro home]] |
{{documentation/{{documentation/version}}/module-introduction-end}} | {{documentation/{{documentation/version}}/module-introduction-end}} | ||
Latest revision as of 02:25, 27 November 2019
Home < Documentation < 4.8 < Modules < AstroSmoothing
For the latest Slicer documentation, visit the read-the-docs. |
Introduction and Acknowledgements
Authors: Contributors: Acknowledgements: Contacts:
|
Module Description
The Smoothing module contain a set of filters (parallelized with OpenMP and OpenGL) aimed to denoise astronomical (HI) dataset:
- Anisotropic Box
- Anisotropic Gaussian
- Intensity-driven Gradient
Panels and their use
References
@ARTICLE{2016A&C....17..163P, author = {{Punzo}, D. and {van der Hulst}, J.~M. and {Roerdink}, J.~B.~T.~M. }, title = "{Finding faint H I structure in and around galaxies: Scraping the barrel}", journal = {Astronomy and Computing}, archivePrefix = "arXiv", eprint = {1609.03782}, primaryClass = "astro-ph.IM", keywords = {Radio lines: galaxies, Techniques: image processing, Scientific visualization}, year = 2016, month = oct, volume = 17, pages = {163-176}, doi = {10.1016/j.ascom.2016.09.002}, }